activity
20042026
most citedSelf-Consistent Models of the AGN and Black Hole Populations: Duty Cycles, Accretion Rates, and the Mean Radiative Efficiency

524 citations · 1.5k across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2026

A Decade-Long Increasing Mid-Infrared Luminosity in Galaxy NGC6447: a Turning-On Candidate of Active Galactic Nucleus

Xinyu Dai, Nate Adams, Natalie Kovacevic +6

It is widely expected that the obscured accretion stage can be the initial turning-on stage of active galactic nuclei from quiescent galaxies. We present mid-infrared light curves…

astro-ph.GA2025

The assembly of supermassive black holes at in early-type galaxies from scaling relations

Duncan Farrah, Athena Engholm, Evanthia Hatziminaoglou +14

The assembly of supermassive black hole (SMBH) mass () and stellar mass () in galaxies can be studied via the redshift evolution of the rela…

astro-ph.HE2023★ 3 cited

Massive black holes in galactic nuclei: Theory and Simulations

Tiziana Di Matteo, Daniel Angles-Alcazar, Francesco Shankar

Massive black holes are fundamental constituents of our cosmos, from the Big Bang to today. Understanding their formation from cosmic dawn, their growth, and the emergence of the f…

astro-ph.GA2022★ 101 cited

The low-end of the black hole mass function at cosmic dawn

Alessandro Trinca, Raffaella Schneider, Rosa Valiante +3

Understanding the formation and growth of supermassive black holes (SMBHs) at high redshift represents a major challenge for theoretical models. In this work we investigate the ear…

astro-ph.CO2013★ 61 cited

Supermassive Black Holes and Their Host Galaxies - II. The correlation with near-infrared luminosity revisited

Ronald Läsker, Laura Ferrarese, Glenn van de Ven +1

We present an investigation of the scaling relations between Supermassive Black Hole (SMBH) masses (Mbh), and their host galaxies' K-band bulge (Lbul) and total (Ltot) luminosities…

astro-ph.CO2013★ 45 cited

Black Hole Demography: From scaling relations to models

Francesco Shankar

In this contributed paper I review our current knowledge of the local Black Hole (BH) scaling relations, and their impact on the determination of the local BH mass function. I part…

astro-ph.CO2011★ 206 cited

Accretion-Driven Evolution of Black Holes: Eddington Ratios, Duty Cycles, and Active Galaxy Fractions

Francesco Shankar, David H. Weinberg, Jordi Miralda-Escude'

We develop semi-empirical models of the supermassive black hole and active galactic nucleus (AGN) populations, which incorporate the black hole growth implied by the observed AGN l…

astro-ph.CO2009★ 110 cited

The Demography of Super-Massive Black Holes: Growing Monsters at the Heart of Galaxies

Francesco Shankar

Supermassive black holes (BHs) appear to be ubiquitous at the center of all galaxies which have been observed at high enough sensitivities and resolution with the Hubble Space Tele…

astro-ph2008★ 106 cited

On the radiative efficiencies, Eddington ratios, and duty cycles of luminous high-redshift quasars

Francesco Shankar, Martin Crocce, Jordi Miralda-Escude' +2

We investigate the characteristic radiative efficiency ε, Eddington ratio λ, and duty cycle P_0 of high-redshift active galactic nuclei (AGN), drawing on measurements of the AGN lu…

astro-ph2007★ 524 cited

Self-Consistent Models of the AGN and Black Hole Populations: Duty Cycles, Accretion Rates, and the Mean Radiative Efficiency

Francesco Shankar, David H. Weinberg, Jordi Miralda-Escude'

We construct evolutionary models of the populations of AGN and supermassive black holes, in which the black hole mass function grows at the rate implied by the observed luminosity…

astro-ph2004★ 352 cited

Super-massive Black Hole Demography: the Match between the Local and Accreted Mass Functions

F. Shankar, P. Salucci, G. L. Granato +2

We have performed a detailed analysis of the local super-massive black-hole (SMBH) mass function based on both kinematic and photometric data and derived an accurate analytical fit…